Craterra

Lunar Valley

A Radial Valley South of Crater Einstein

Extending due south of the crater Einstein, Vallis Bohr is a wide cleft formed by secondary craters from the Orientale impact.

Feature Profile & Selenographic Data

Feature type
vallis
Coordinates
10.25° N · 88.86° W
Diameter
95.32 km
IAU approval
1976/01/01 00:00:00
LAC quadrangle
LAC-55 · Vasco da Gama

Geological Chronicle

Vallis Bohr is a wide lunar cleft stretching due south of the crater Einstein, with a length of about 80 kilometers.

Radial to Mare Orientale farther to the south, the valley is a chain of secondary craters produced by the Orientale impact.

Scientific Sources & References

Name Origin

Named from nearby crater.

Interactive Lunar Surface

Explore Vallis Bohr in 3D

Inspect lunar elevation data and the official selenographic position.